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Paper Citation Record · LEDGER

The initial value problem as it relates to numerical relativity

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1610.03805.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
1610.03805 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T05:28:09.076903Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-08-07T11:41:20.669697Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 5079398d-c5de-4236-a591-b50f433caff4 · inbound

Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung cites this paper.

Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung The initial value problem as it relates to numerical relativity

Reference 72

Resolution
unresolved
no resolver link, observed 2026-08-14T05:28:09.076903Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T05:28:09.076903Z digest=sha256:6356a8d828347a463f529af92f36ecc8494948281f8b783ea6193656905c3aa5

Observation 7ef06415-affe-4611-a583-f67924e81b6a · inbound

The error budget of binary neutron star merger simulations for configurations with high spin cites this paper.

The error budget of binary neutron star merger simulations for configurations with high spin The initial value problem as it relates to numerical relativity

Reference 140

Resolution
verified exact
local_arxiv, observed 2026-08-07T11:41:20.706507Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-08-07T11:40:59.733254Z digest=sha256:54e2c6fb1bcbc60437bebca369ef72361c437b0d72ddc7ea0ec280987b195642